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20 April 2024
 
  » arxiv » astro-ph/0206001

 Article overview


System description and first light-curves of HAT, an autonomous observatory for variability search
Gaspar A. Bakos ; Jozsef Lazar ; Istvan Papp ; Pal Sari ; Elizabeth M. Green ;
Date 31 May 2002
Subject astro-ph
AffiliationCfA and Konkoly Obs.), Jozsef Lazar (Hungarian Astronomical Association, HAA), Istvan Papp (HAA), Pal Sari (HAA), Elizabeth M. Green (Steward Obs., Univ. of Arizona
AbstractHaving been operational at Kitt Peak for more than a year, the prototype of the Hungarian Automated Telescope (HAT-1) has been used for all-sky variability search of the northern hemisphere. The small autonomous observatory is recording brightness of stars in the range of I~6--13m with a telephoto lens and its 9x9 degree field of view, yielding a data rate of ~10^6 photometric measurements per night. We give brief hardware and software description of the system, controlled by a single PC running RealTime Linux operating system. We overview site-specific details, and quantify the astrometric and photometric capabilities of HAT. As a demonstration of system performance we give a sample of 60 short period variables in a single selected field, all bright, with I < 13m, of which only 14 were known before. Depending on the observing strategy, search for extrasolar planet transits is also a feasible observing program. We conclude with a short discussion on future directions. Further information can be found at the HAT homepage: http://www-cfa.harvard.edu/~gbakos/HAT/
Source arXiv, astro-ph/0206001
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